Detection limits at 5σ for IRDIS in the K1 band on the left and IFS in the YJH bands on the right. Data are reduced at the top by the pipeline SpeCal-TLOCI (for IRDIS) or SpeCal-PCAPad (for IFS) and at the bottom by the pipeline ANDROMEDA. The gray area corresponds to the area hidden by the larger coronagraph used for all the epochs (i.e., N_ALC_Ks) which has an inner working angle of 0.107″ and 0.116″ for IFS and IRDIS, respectively. The blue vertical line corresponds to the position of the planet HD 95086 b at the best epoch January 2018 (cyan, 0.625″).